Report
The multiple merger assembly of a hyperluminous obscured quasar at redshift 4.6
- T. Díaz-Santos1,*,
- R. J. Assef1,
- A. W. Blain2,
- M. Aravena1,
- D. Stern3,
- C.-W. Tsai4,
- P. Eisenhardt3,
- J. Wu5,
- H. D. Jun6,
- K. Dibert7,
- H. Inami8,
- G. Lansbury9,
- F. Leclercq8
- 1Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Ejército Libertador 441, Santiago, 8320000, Chile.
- 2Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK.
- 3Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
- 4Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095, USA.
- 5National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China.
- 6School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, Seoul 02455, Korea.
- 7Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA.
- 8Université Lyon, Université Lyon1, École Normale Supérieure de Lyon, Centre National de la Recherche Scientifique, Centre de Recherche Astrophysique de Lyon UMR5574, 69230 Saint-Genis-Laval, France.
- 9Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK.
- ↵*Corresponding author. Email: tanio.diaz{at}mail.udp.cl
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Science 30 Nov 2018:
Vol. 362, Issue 6418, pp. 1034-1036
DOI: 10.1126/science.aap7605
